Quantization of the Reissner-Nordstr\"{o}m Black Hole
P. Breitenlohner (Munich, Max Planck Inst.), H. Hollmann (Cambridge,, DAMTP), D. Maison (Munich, Max Planck Inst.)

TL;DR
This paper applies group theoretical quantization to the Reissner-Nordström black hole, deriving spectra of observables within a sigma model framework coupled to Euclidean gravity.
Contribution
It introduces a novel group theoretical quantization approach for Reissner-Nordström black holes within a sigma model context, identifying key observables and their spectra.
Findings
Spectra of observables are explicitly calculated.
Reissner-Nordström solutions are connected to a nonlinear sigma model.
Quantization provides new insights into black hole properties.
Abstract
The Reissner--Nordstr\"{o}m family of solutions can be understood to arise from the spherically symmetric sector of a nonlinear SO(2,1)/SO(1,1) sigma model coupled to three dimensional Euclidean gravity. In this context a group theoretical quantization is performed. We identify the observables of the theory and calculate their spectra.
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